Stellar cluster and star-forming region M 17 (annotated)

Three-colour composite of the sky region of M 17, a H II region excited by a cluster of young, hot stars. A large silhouette disc has been found to the south-west of the cluster centre. The present image was obtained with the ISAAC near-infrared instrument at the 8.2-m VLT ANTU telescope at Paranal. The orientation and the scale at the distance of M 17 (7,000 light-years) are indicated, and the main regions are identified.

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Om bilden

ID:eso0416b
Typ:Observation
Publiceringsdatum:12 maj 2004
Relaterade pressmeddelanden:eso0416
Storlek:773 x 772 px

Om objektet

Namn:Messier 17, Omega Nebula
Typ:Milky Way : Nebula : Appearance : Emission : H II Region
Milky Way : Nebula : Type : Star Formation
Avstånd:5500 ljusår
Constellation:Sagittarius
Kategori:Star Clusters

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Stor jpeg
270,6 kB
Skärmstor jpeg
315,5 kB

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1600x1200
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1920x1200
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2048x1536
751,5 kB

Koordinater

Position (RA):18 20 47.06
Position (Dec):-16° 10' 19.25"
Field of view:6.03 x 6.02 arcminutes
Orientering:Nord är 0.1° vänster om lodrätt

Färger och filter

BandVåglängdTeleskop
Infrarött
J
1.25 μmVery Large Telescope
ISAAC
Infrarött
H
1.6 μmVery Large Telescope
ISAAC
Infrarött
K
2.2 μmVery Large Telescope
ISAAC